Observational constraints on teleparallel effective equation of state
A cluster of astronomical observations emerged that the present Universe is in a phase of
accelerated expansion. To examine the accelerated expansion of the Universe, we used the …
accelerated expansion. To examine the accelerated expansion of the Universe, we used the …
Noncompactified Kaluza–Klein Gravity
We present a brief description of noncompactified higher-dimensional theories from the
perspective of general relativity. More concretely, the Space–Time–Matter theory, or Induced …
perspective of general relativity. More concretely, the Space–Time–Matter theory, or Induced …
Anisotropic compact stars in f(G) gravity
This paper is devoted to study the possibility of forming anisotropic compact stars in modified
Gauss–Bonnet, namely called as f (G) theory of gravity which is one of the strong …
Gauss–Bonnet, namely called as f (G) theory of gravity which is one of the strong …
Bianchi type-III cosmological model in f(R,T) theory of gravity
DRK Reddy, R Santikumar, RL Naidu - Astrophysics and Space Science, 2012 - Springer
A spatially homogeneous Bianchi type-III space-time is considered in the presence of perfect
fluid source in the frame work of f (R, T) gravity (Harko et al. in Phys. Rev. D 84: 024020 …
fluid source in the frame work of f (R, T) gravity (Harko et al. in Phys. Rev. D 84: 024020 …
Cosmological models with a hybrid scale factor in an extended gravity theory
A general formalism to investigate Bianchi type VI h universes is developed in an extended
theory of gravity. A minimally coupled geometry and matter field is considered with a …
theory of gravity. A minimally coupled geometry and matter field is considered with a …
Axially symmetric cosmological model in f (R, T) gravity
An axially symmetric space-time is considered in the presence of a perfect fluid source in the
framework of f (R, T) gravity, where R is the Ricci scalar and T is the trace of the energy …
framework of f (R, T) gravity, where R is the Ricci scalar and T is the trace of the energy …
A new class of Bianchi cosmological models in f(R,T) gravity
The new class of cosmological model of the early Universe is considered with f (R, T)
modified theories of gravity (Harko et al. in Phys. Rev. D 84: 024020, 2011). The exact …
modified theories of gravity (Harko et al. in Phys. Rev. D 84: 024020, 2011). The exact …
A generalized Buchdahl model for compact stars in f (R, T) gravity
In this paper, we study the stellar structure in terms of alternative theory of gravity specially
by f (R, T) gravity theory. Here, we consider the function f (R, T)= R+ 2 ς T where R is the …
by f (R, T) gravity theory. Here, we consider the function f (R, T)= R+ 2 ς T where R is the …
Bianchi type-III Dark Energy Model in f(R,T) Gravity
DRK Reddy, R Santhi Kumar… - International Journal of …, 2013 - Springer
A dark energy model with EoS parameter is investigated in f (R, T) gravity in Bianchi type-III
space-time in the presence of perfect fluid source. To obtain a determinate solution special …
space-time in the presence of perfect fluid source. To obtain a determinate solution special …
Dynamics of the anisotropic Kantowsky–Sachs geometries in Rn gravity
We construct general anisotropic cosmological scenarios governed by an f (R) gravitational
sector. Focusing then on Kantowski–Sachs geometries in the case of R n-gravity, and …
sector. Focusing then on Kantowski–Sachs geometries in the case of R n-gravity, and …